The 1 g voyage: the maths
Special relativity for a ship with constant proper acceleration (what the crew feels), accelerating to halfway and braking the rest. Computed live.
Equations
- τ = (2c/g) · arcosh(1 + gD / 2c²)
- Time on the ship's clock for a trip of distance D.
- T = (2c/g) · sinh(gτ / 2c)
- Time on Earth's clock for the same trip.
- vmax = c · tanh(gτ / 2c)
- Top speed, at the halfway point.
Constants
| g | 9.80665 m/s² ≈ 1.032 light-years per year² | standard gravity |
| light-year | 9.4607304725808 × 10¹⁵ m | exact |
Worked examples ✓ checked on every change
| Proxima Centauri (4.24 ly) at 1 g: the crew's time | 3.54 years | the formula above |
| …and Earth's time | 5.90 years | the commonly quoted 5.9 years |
| Centre of the galaxy (26,000 ly): the crew's time | 19.8 years | the formula above |
What's simplified
- No fuel limit: the ship is a perfect photon rocket (the fuel ratio shows what that would still cost).
- No dust, radiation or time to turn round.
Where it breaks
Never, for the kinematics — this is exact special relativity. Only the engineering is imaginary.
Sources: C. Misner, K. Thorne & J. Wheeler, Gravitation (1973), §6; J. Baez, 'The Relativistic Rocket' (Usenet Physics FAQ).